Exact Space-Times in Einstein's General Relativity: Friedmann–Lemaître–Robertson–Walker space-times

By J. Griffiths, J. Podolský. 2009

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The Weak Gravity Conjecture in three dimensions (2016, background): “This means that one can build charged black hole solutions (the Reissner-Nordstron metric [32, 33] and its higher-dimensional cousins, black branes of dimension d − 3) and the metric is sensitive to the electric field of the black hole.”
The classical double copy in maximally symmetric spacetimes (2017, methodology): “The case of de Sitter pp-waves is identical to the Kundt waves analyzed above [62]; thus, here we will only consider the AdS case.”
Regular Black Holes: A Short Topic Review (2023, background): “Let us see the well-known Taub-NUT BH [84,85] as a sample,”
Photon regions and shadows of accelerated black holes (2015, background): “d) circles are the celestial equator = ˇ=2 and its image under stereographic projection. The second equation denes the celestial coordinates and , see Fig. 4. For the scalar factor ˙we obtain with (15) ˙= g ;e_ 0 = aLz ( + a˜)E p r (r O;# O) : (26) We substitute _’and _rfrom (16b) and (16d) into (24”
Type D spacetimes and the Weyl double copy (2018, unknown): “15) 3See [84] or [85] for more details on this classification.”